Relation of X-ray activity and rotation in M dwarfs and predicted time-evolution of the X-ray luminosity

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Volume 638 (June 2020)

A&A, 638 (2020) A20

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Table B.1.

Stellar parameters and updated X-ray results we computed for the 288 stars we took from the literature samples (Wright et al. 2011, 2018; Wright & Drake 2016; Stelzer et al. 2016; González-Álvarez et al. 2019).

Name	M_{K_s}	M_⋆	R_⋆		V − J	P_rot	log(L_x)		R_O, C&S	R_O, B	R_O, W	D	FLAG_GAIA
	[mag]	[M_⊙]	[R_⊙]		[mag]	[d]	[erg/s]					[pc]
HAT 122−01032	6.33±0.03	0.41±0.01	0.40±0.01	−1.73±0.04	4.26	4.38	28.91±0.01	−2.94±0.09	–	–	0.05	18.63±0.03	1 1
LP 149−56	5.85±0.03	0.49±0.01	0.47±0.01	−1.51±0.04	3.71	6.17	28.84±0.03	−3.24±0.10	0.14	0.25	0.10	29.56±0.05	1 1
G 172−1	7.14±0.10	0.30±0.01	0.29±0.01	−2.06±0.19	4.32	1.09	28.72±0.04	−2.81±0.23	–	–	0.01	14.77±0.71	0 1
UCAC4 729−006249	5.14±0.03	0.61±0.01	0.59±0.02	−1.16±0.03	2.80	8.35	29.09±0.03	−3.33±0.10	0.24	0.45	0.23	43.63±0.07	1 1
2MASS J00380001+4353454	4.24±0.16	0.76±0.03	0.76±0.04	−0.81±0.12	2.95	0.55	29.91±0.03	−2.87±0.34	0.01	0.07	0.01	97.19±1.32	1 1
1RXS J003926.5+381607	4.48±0.16	0.72±0.03	0.71±0.04	−0.89±0.13	2.77	3.08	29.36±0.12	−3.33±0.35	0.09	0.26	0.09	115.40±1.59	1 1
...	...	...	...	...	...	...	...	...	...	...	...	...	...
...	...	...	...	...	...	...	...	...	...	...	...	...	...

Notes. The last column shows the FLAG we used to verify if Gaia distances are reliable as explained in Sect. 3. The full table is available in electronic form at the CDS.

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